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Paper Citation Record · LEDGER

Classification of magnetized star--planet interactions: bow shocks, tails, and inspiraling flows

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1503.03551.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1503.03551 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T15:25:39.373394Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-06T15:25:40.551695Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 760a0c90-fee4-4602-8002-73f26fe9f6e9 · inbound

A Self-Consistent 3D Hydrodynamic Model for Helium Transit Signatures in Evaporating Hot Jupiters cites this paper.

A Self-Consistent 3D Hydrodynamic Model for Helium Transit Signatures in Evaporating Hot Jupiters Classification of magnetized star--planet interactions: bow shocks, tails, and inspiraling flows

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-01T15:45:56.929558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T15:45:56.929558Z digest=sha256:d1a4e0a3f7e9710bf67fdef800377d40b6254c4a23cf6a38cc7402031910ddb7

Observation 9985f83f-7a30-4c05-acb5-f711d463ad45 · inbound

Circular polarization as a probe of cloud properties and asymmetries in giant exoplanet atmospheres cites this paper.

Circular polarization as a probe of cloud properties and asymmetries in giant exoplanet atmospheres Classification of magnetized star--planet interactions: bow shocks, tails, and inspiraling flows

Reference 83

Resolution
verified exact
local_arxiv, observed 2026-08-06T15:25:40.555544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-08-06T15:25:39.373394Z digest=sha256:9e64efbed1e69c17577c4d0a2dad0324a95b98facc37afb1df4832655f85136d